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Nature and origin of matrix in the unique type 3 chondrite, KakangariThe characteristics of the matrix of the Kakangari type-3 chondrite were investigated using high-resolution TEM and AEM. It was found that the textural and mineralogical characteristics of the fine-grained matrix of Kakangari are different from those of the other chondrite groups. Unlike the matrix phases present in the CV3 and CO3 chondrites, the matrix mineralogy of Kakangari contains clear information regarding its possible origin and thermal history. Data obtained are most consistent with an origin of Kakangari by annealing, without melting at high temperature (possibly during a chondrule-forming thermal event), of clusters or aggregates of ultrafine-grained amorphous or crystalline phases. The precursor materials were most likely to have been a mixture of nebula and presolar dust. Chondrules in Kakangari were probably formed from identical precursors to the matrix, but reached temperatures sufficiently high to produce melting.
Document ID
19890066930
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Brearley, Adrian J.
(New Mexico, University Albuquerque, United States)
Date Acquired
August 14, 2013
Publication Date
September 1, 1989
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 53
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
89A54301
Funding Number(s)
CONTRACT_GRANT: NAG9-30
Distribution Limits
Public
Copyright
Other

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